{"id":3773,"date":"2026-04-20T03:48:51","date_gmt":"2026-04-20T03:48:51","guid":{"rendered":"https:\/\/terrarara.com.br\/en\/?page_id=3773"},"modified":"2026-04-20T03:48:51","modified_gmt":"2026-04-20T03:48:51","slug":"o-fluxo-escuro-o-enigma-cosmico-que-puxa-galaxias-para-alem-do-visivel","status":"publish","type":"page","link":"https:\/\/terrarara.com.br\/en\/?page_id=3773","title":{"rendered":"The dark stream: the cosmic enigma pulling galaxies beyond the visible"},"content":{"rendered":"
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Hot gas in moving galaxy clusters (white spots) shifts the temperature of cosmic microwaves. Hundreds of distant clusters seem to be moving toward one patch of sky (purple ellipse). Credit: NASA\/WMAP\/A. Kashlinsky et al.<\/figcaption><\/figure><\/div>
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\r\nIn 2008, a team of astronomers led by Alexander Kashlinsky of NASA’s Goddard Space Flight Center made a surprising discovery while analyzing data from the Wilkinson Microwave Anisotropy Probe (WMAP) satellite<\/strong><\/p>

They identified an unexpected collective movement in hundreds of distant galaxy clusters, something that didn’t fit the predictions of traditional cosmological models.<\/p>

\r\nDubbed the “dark stream,” this phenomenon reveals that entire galaxy clusters are moving at high speed toward a specific region of the sky, as if drawn by a gravitational force from something beyond the observable universe.\r\n<\/p>

\r\nThe dark stream was detected thanks to a subtle effect called the kinematic Sunyaev-Zel’dovich effect.<\/p>

\r\nHot gas within galaxy clusters scatters photons from the cosmic microwave background-that ancient light emitted about 380,000 years after the Big Bang, which serves as the definitive reference for the large-scale motion of the universe.<\/p>

\r\nAs the clusters move relative to this background, the wavelengths of the photons shift slightly, creating a small temperature variation in the microwave map.<\/p>

\r\nOn its own, the effect is too weak to be seen in a single cluster, but by studying a large number of them-about 700 objects reaching distances of up to 6 billion light-years-researchers were able to amplify the signal and reveal the mass movement.\r\n<\/p>

\r\nThe results were impressive: the clusters are moving at nearly 3.2 million kilometers per hour (about 2 million miles per hour) toward an area of “”approximately 20 degrees in the sky, located between the constellations Centaurus and Vela.<\/p>

\r\nThe most intriguing aspect is that this flow doesn’t diminish with distance, as would be expected if it were caused solely by visible matter within our universe.<\/p>

\r\nOn the contrary, it remains constant for billions of light-years, suggesting that the distribution of matter as we know it simply cannot explain what is happening.<\/p>

\r\n“We never expected to find something like this,” Kashlinsky stated at the time.\r\n<\/p>

\r\nFive years later, in 2013, the same team published even more surprising results.<\/p>

\r\nUsing more precise data from WMAP (the five-year mission) and doubling the number of clusters analyzed, they were able to trace the dark flow to twice the original distance, reaching regions about 2.5 billion light-years from Earth.<\/p>

\r\nThe movement continues to point in the same general direction, now associated with the constellations Centaurus and Hydra, and persists with the same intensity.<\/p>

\r\nThe team, which included researchers such as Fernando Atrio-Barandela, Harald Ebeling, and Alastair Edge, divided the clusters into “slices” of different distances and confirmed that the pattern repeats consistently.<\/p>

\r\nThe brightest clusters in X-rays-those with the most hot gas-showed the strongest effect, reinforcing that the signal was not mere statistical noise.\r\n<\/p>

\r\nThis persistence of the dark flow challenges conventional theories.<\/p>

\r\nAccording to cosmologists, the cosmic microwave background represents the “frame of reference” of the universe: in relation to it, there should be no preferential large-scale movement.<\/p>

\r\nHowever, what is observed is exactly the opposite.<\/p>

\r\nThe most plausible explanation, according to the researchers, refers to the period of cosmic inflation-that hyper-rapid expansion that the universe experienced shortly after the Big Bang.<\/p>

\r\nIf inflation really occurred, the universe we see is only a small part of a much larger cosmos.<\/p>

\r\nMatter that was pushed far beyond our observable horizon could be exerting a gravitational pull on our neighborhood, creating this mysterious flow.\r\n<\/p>

\r\nScientists compare the dark flow to other great mysteries, such as dark matter and dark energy.<\/p>

\r\n“The distribution of matter in the observed universe cannot explain this movement,” Kashlinsky emphasizes.<\/p>

\r\nThe discovery opens a fascinating window to explore the state of the cosmos even before inflation.<\/p>

\r\nAlthough controversial and not yet confirmed by all models, the dark stream continues to be investigated with data from missions such as Planck, from the European Space Agency, which maps the microwave background with even greater precision.\r\n<\/p>

\r\nTo this day, the phenomenon intrigues the scientific community because it suggests that the visible universe is only the tip of a much larger cosmic iceberg.<\/p>

\r\nWhat pulls these galaxy clusters together may be hidden in regions we will never be able to see directly, but whose effects we feel through gravity.<\/p>

\r\nFuture studies, with larger catalogs of clusters and more refined analyses of the hot gas, promise to reduce uncertainties and perhaps reveal whether the dark stream is indeed a sign of a multiverse or something even more extraordinary.<\/p>

\r\nFor now, it remains a humble reminder that the cosmos holds profound secrets, waiting to be deciphered by the next generations of telescopes and space observatories.

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Published in 04\/20\/2026 03h48<\/em><\/p>\r\n

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Portuguese version<\/a><\/em><\/p>\r\n

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Text adapted by AI (Grok) and translated via Google API in the English version. Images from public image libraries or credits in the caption. Information about DOI, author and institution can be found in the body of the article.<\/p>\r\n\t\t

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Reference article:<\/p>\r\n\t\t\r\n\t\t\r\n\r\n\r\n